The Astrophysical Journal (Jan 2024)

UNCOVER: A NIRSpec Census of Lensed Galaxies at z = 8.50–13.08 Probing a High-AGN Fraction and Ionized Bubbles in the Shadow

  • Seiji Fujimoto,
  • Bingjie Wang,
  • John R. Weaver,
  • Vasily Kokorev,
  • Hakim Atek,
  • Rachel Bezanson,
  • Ivo Labbe,
  • Gabriel Brammer,
  • Jenny E. Greene,
  • Iryna Chemerynska,
  • Pratika Dayal,
  • Anna de Graaff,
  • Lukas J. Furtak,
  • Pascal A. Oesch,
  • David J. Setton,
  • Sedona H. Price,
  • Tim B. Miller,
  • Christina C. Williams,
  • Katherine E. Whitaker,
  • Adi Zitrin,
  • Sam E. Cutler,
  • Joel Leja,
  • Richard Pan,
  • Dan Coe,
  • Pieter van Dokkum,
  • Robert Feldmann,
  • Yoshinobu Fudamoto,
  • Andy D. Goulding,
  • Gourav Khullar,
  • Danilo Marchesini,
  • Michael Maseda,
  • Themiya Nanayakkara,
  • Erica J. Nelson,
  • Renske Smit,
  • Mauro Stefanon,
  • Andrea Weibel

DOI
https://doi.org/10.3847/1538-4357/ad9027
Journal volume & issue
Vol. 977, no. 2
p. 250

Abstract

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We present JWST NIRSpec prism spectroscopy of lensed galaxies at z ≳ 9 found behind the massive galaxy cluster Abell 2744 in the UNCOVER Cycle 1 Treasury Program. We confirm the redshift via emission lines and/or the Ly α break for 10 galaxies at z = 8.50–13.08 down to M _V = −17.3. We achieve a 100% confirmation rate for z > 9 candidates reported in H. Atek et al. Using six sources with multiple line detections, we find that offsets in redshift estimates between the lines and the Ly α break alone can be ±0.2, raising caution in designing future follow-up spectroscopy for the break-only sources with the Atacama Large Millimeter/submillimeter Array. With spec- z -confirmed sources in UNCOVER and the literature, we derive lower limits on the rest-frame ultraviolet (UV) luminosity function (LF) at z ≃ 9–12 and find that these lower limits agree with recent photometric measurements. We identify at least two unambiguous and several possible active galactic nucleus (AGN) systems based on X-ray, broad H β , high ionization lines, and excess in the UV LF. This requires the AGN LFs at z ≃ 9–10 to be comparable or even higher than the X-ray AGN LF estimated at z ∼ 6 and suggests a plausible cause of the high abundance of z > 9 galaxies claimed in the recent photometric measurements is AGNs. One UV-luminous source is confirmed at the same redshift as a broad-line AGN at z = 8.50 with a physical separation of 380 kpc in the source plane. These two sources show emission blueward of Ly α , indicating a giant ionized bubble enclosing them with a radius of 7.69 ± 0.18 pMpc. Our results imply that AGNs have a nonnegligible contribution to cosmic reionization.

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